Fused silica suspension for the VIRGO optics: status and perspectives

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Published 14 March 2002 Published under licence by IOP Publishing Ltd
, , Citation P Amico et al 2002 Class. Quantum Grav. 19 1669 DOI 10.1088/0264-9381/19/7/359

0264-9381/19/7/1669

Abstract

Thermal noise in mirror suspension wires is the main limitation of low-frequency sensitivity of interferometric gravitational wave detectors. In order to minimize the pendulum thermal noise, a monolithic design, using a low dissipation material, is proposed for VIRGO. High mechanical Qs and high breaking strengths have been obtained for monolithic fused silica fibres. A low-dissipation and high-strength bonding technique using potassium silicate bonding is proposed.

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10.1088/0264-9381/19/7/359